In situ detection of water on the Moon by the Chang’E-5 lander

Author:

Lin Honglei1ORCID,Li Shuai2ORCID,Xu Rui3ORCID,Liu Yang45ORCID,Wu Xing4ORCID,Yang Wei1ORCID,Wei Yong1ORCID,Lin Yangting1ORCID,He Zhiping3ORCID,Hui Hejiu56ORCID,He Huaiyu1,Hu Sen1ORCID,Zhang Chi1ORCID,Li Chunlai3ORCID,Lv Gang3,Yuan Liyin3,Zou Yongliao4,Wang Chi4ORCID

Affiliation:

1. Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, PR China.

2. Hawaii Institute of Geophysics and Planetology, University of Hawaiʻi at Mānoa, Honolulu, HI, USA.

3. Key Laboratory of Space Active Opto-Electronics Technology, Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, PR China.

4. State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, PR China.

5. Center for Excellence in Comparative Planetology, Chinese Academy of Sciences, Hefei 200083, PR China.

6. State Key Laboratory for Mineral Deposits Research and Lunar and Planetary Science Institute, School of Earth Sciences and Engineering, Nanjing University, Nanjing 210023, PR China.

Abstract

Variations of total water contents were detected in situ from the lunar regolith and rock at the Chang’E-5 landing site.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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